A compact multi-planet system transiting HIP 29442 (TOI-469) discovered by TESS and ESPRESSO - Radial velocities lead to the detection of transits with low signal-to-noise ratio

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Fig. 7

TESS PDCSAP light curve with the GP component subtracted, and phase-folded to the orbital periods of HIP 29442 b (first panel), HIP 29442 c (second panel), and HIP 29442 d (third panel). The solid lines indicate the models calculated using the median of the posteriors. Residuals of the best-fit model are shown at the bottom of each phase-folded plot.

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